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The inner pair orbit each other with a period of 26.8 years, a semimajor axis of 0.33 arc seconds, and an eccentricity of 0.515. They have a blended stellar classification of A7 IV, matching a white-hued A-typesubgiant star. Both stars are actual A-type main sequence stars. The brighter of the pair, magnitude 5.20 component A, has a spectral class of A4 V, while its magnitude 5.76 companion, component B, is of class A6 V. The two are 1.94 and 1.65 times as massive as the Sun, respectively. The tertiary member, component C, is a magnitude 8.1 star with 0.88 times the mass of the Sun. It lies at an angular separation of 10.8 arc seconds from the other members.
^ David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146, S2CID33401607.